3.6k citations · 12.1k across the 20 of their papers we have counts for
59 papers
Long Range Plan: Dense matter theory for heavy-ion collisions and neutron stars
Alessandro Lovato, Travis Dore, Robert D. Pisarski +61
Since the release of the 2015 Long Range Plan in Nuclear Physics, major events have occurred that reshaped our understanding of quantum chromodynamics (QCD) and nuclear matter at l…
Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
Marcella Wijngaarden, Katerina Chatziioannou, Andreas Bauswein +2
The gravitational wave signal emitted during the coalescence of two neutron stars carries information about the stars' internal structure. During the long inspiral phase the main m…
Impact of the PSR J0740+6620 radius constraint on the properties of high-density matter
Isaac Legred, Katerina Chatziioannou, Reed Essick +2
X-ray pulse profile modeling of PSR J0740+6620, the most massive known pulsar, with data from the NICER and XMM-Newton observatories recently led to a measurement of its radius. We…
A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
Katerina Chatziioannou, Maximiliano Isi, Carl-Johan Haster +1
Gravitational waves in general relativity contain two polarization degrees of freedom, commonly labeled plus and cross. Besides those two tensor modes, generic theories of gravity…
Modeling compact binary signals and instrumental glitches in gravitational wave data
Katerina Chatziioannou, Neil Cornish, Marcella Wijngaarden +1
Transient non-gaussian noise in gravitational wave detectors, commonly referred to as glitches, pose challenges for inference of the astrophysical properties of detected signals wh…
Prospects of gravitational-waves detections from common-envelope evolution with LISA
M. Renzo, T. Callister, K. Chatziioannou +6
Understanding common envelope (CE) evolution is an outstanding problem in binary evolution. Although the CE phase is not driven by gravitational-wave (GW) emission, the in-spiralin…